TeraHertz Exploration and Zooming-in for Astrophysics (THEZA): ESA Voyage 2050 White Paper

(2019)

Authors:

Leonid I Gurvits, Zsolt Paragi, Viviana Casasola, John Conway, Jordy Davelaar, Heino Falcke, Rob Fender, Sándor Frey, Christian M Fromm, Cristina García Miró, Michael A Garrett, Marcello Giroletti, Ciriaco Goddi, José-Luis Gómez, Jeffrey van der Gucht, José Carlos Guirado, Zoltán Haiman, Frank Helmich, Elizabeth Humphreys, Violette Impellizzeri, Michael Kramer, Michael Lindqvist, Hendrik Linz, Elisabetta Liuzzo, Andrei P Lobanov, Yosuke Mizuno, Luciano Rezzolla, Freek Roelofs, Eduardo Ros, Kazi LJ Rygl, Tuomas Savolainen, Karl Schuster, Tiziana Venturi, Martina Wiedner, J Anton Zensus

A new sample of southern radio galaxies: host-galaxy masses and star-formation rates

Monthly Notices of the Royal Astronomical Society Oxford University Press 489:3 (2019) 3403-3411

Authors:

T Marubini, Matthew Jarvis, S Fine, T Mauch, K McAlpine, M Prescott

Automatic selection of correlated double sampling timing parameters

Journal of Astronomical Telescopes, Instruments, and Systems Society of Photo-optical Instrumentation Engineers 5:4 (2019)

Authors:

Daniel Weatherill, Ian Shipsey, Kirk Arndt, Richard Plackett, Daniel Wood, Kaloyan Metodiev, Maria Mironova, Daniela Bortoletto, N Demetriou

Abstract:

Correlated double sampling (CDS) is a process used in many charge-coupled device readout systems to cancel the reset noise component that would otherwise dominate. CDS processing typically consists of subtracting the integrated video signal during a “signal” period from that during a “reset” period. The response of this processing depends, therefore, on the shape of the video signal with respect to the integration bounds. In particular, the amount of noise appearing in the final image and the linearity of the pixel value with signal charge are affected by the choice of the CDS timing intervals. We use a digital CDS readout system which highly oversamples the video signal (as compared with the pixel rate) to reconstruct pixel values for different CDS timings using identical raw video signal data. We use this technique to develop insights into optimal strategy for selecting CDS timings both in the digital case (where the raw video signal may be available) and in the general case (where it is not). In particular, we show that the linearity of the CDS operation allows subtraction of the raw video signals of pixels in bias images from those in illuminated images to directly show the effects of CDS processing on the final (subtracted) pixel values.

Search for supersymmetry in final states with two same-sign or three leptons and jets using 36 fb(-1) of root s = 13 TeV pp collision data with the ATLAS detector (vol 09, 084, 2017)

JOURNAL OF HIGH ENERGY PHYSICS 2019:8 (2019) ARTN 121

Authors:

M Aaboud, G Aad, B Abbott, Dc Abbott, O Abdinov, B Abeloos, Dk Abhayasinghe, Sh Abidi, Os AbouZeid, Nl Abraham, H Abramowicz, H Abreu, Y Abulaiti, Bs Acharya, S Adachi, L Adam, L Adamczyk, L Adamek, J Adelman, M Adersberger, A Adiguzel, T Adye, Aa Affolder, Y Afik, C Agheorghiesei, Ja Aguilar-Saavedra, F Ahmadov, G Aielli, S Akatsuka, Tpa Akesson, E Akilli, Av Akimov, Gl Alberghi, J Albert, P Albicocco, Mj Alconada Verzini, S Alderweireldt, M Aleksa, In Aleksandrov, C Alexa, D Alexandre, T Alexopoulos, M Alhroob, B Ali, G Alimonti, J Alison, Sp Alkire, C Allaire, Bmm Allbrooke, Bw Allen

Abstract:

© 2019, The Author(s). One correction is made to the figure 4e of the paper.

Statistical properties of polarized CMB foreground maps

Monthly Notices of the Royal Astronomical Society Oxford University Press (OUP) 487:4 (2019) 5814-5823

Authors:

Sebastian von Hausegger, Aske Gammelgaard Ravnebjerg, Hao Liu